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Proposal of Temperature Correction of Molten Oxide Based on Its Emissivity for Measurement of Temperature Dependence of Its Density Using ELF in ISS
Gakushuin Univ, Dept Phys, Tokyo, Japan..
Gakushuin Univ, Dept Phys, Tokyo, Japan..
Gakushuin Univ, Dept Phys, Tokyo, Japan..
Gakushuin Univ, Dept Phys, Tokyo, Japan..
Vise andre og tillknytning
2023 (engelsk)Inngår i: INTERNATIONAL JOURNAL OF MICROGRAVITY SCIENCE AND APPLICATION, ISSN 0915-3616, Vol. 40, nr 1, artikkel-id 400101Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We determined the emissivity of molten oxides using a commercially available pyrometer combined and an electromagnetic levitation system based on the liquid Fe emissivity and its melting temperature. Our method for determining molten oxide emissivity is based on immiscible molten oxides and liquid Fe. From the processes, we obtained 0.80 +/- 0.03 for molten Al2O3 and 0.76 +/- 0.01 for our de-sired molten oxide of SiO2-CaO-Mn3O4-TiO2 system with welding flux model compositions of SiO2:CaO:Mn3O4:TiO2=27:7:13:53 mass%. This is necessary when using ELF (electrostatic levitation furnace) in the ISS (International Space Station) to measure the thermophysical prop-erties of molten oxides. We could correct the monitored with emissivity set at 1 to the real temperature during density measurement by ELF in ISS using normal spectral emissivity for molten SiO2-CaO-Mn3O4-TiO2 system and we find the temperature dependence of molten oxides den-sity of SiO2:CaO:Mn3O4:TiO2=27:7:13:53 mass% in the temperature range of 1200 K -2000 K. We also find that the multicomponent oxide system of SiO2-CaO-Mn3O4-TiO2 has a low coefficient of density temperature dependence.

sted, utgiver, år, opplag, sider
The Japan Society of Microgravity Application , 2023. Vol. 40, nr 1, artikkel-id 400101
Emneord [en]
Emissivity, Molten Oxide, Density, Container-less Technique, Levitation
HSV kategori
Identifikatorer
URN: urn:nbn:se:hj:diva-60982DOI: 10.15011/jasma.40.400101ISI: 000990114000002Lokal ID: GOA;intsam;884748OAI: oai:DiVA.org:hj-60982DiVA, id: diva2:1765079
Tilgjengelig fra: 2023-06-09 Laget: 2023-06-09 Sist oppdatert: 2023-06-09bibliografisk kontrollert

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